This file contains the Asteroid
Polarimetry Database (APD) compiled by D.F. Lupishko and S.V. Vasilyev
of Karazin Kharkiv National University, Ukraine. It contains the
majority of asteroid polarimetry published by Feb. 10, 2014. The APD
includes data in the form of complete polarization curves (degree of
polarization vs. phase angle) as well as the polarization and position
angle reduced to the proper coordinate system, where available.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
LAP DISTURBANCE OCCURRING AT CONSTANT FREQUENCIES HAS BEEN ELIMINATED.
DYNAMIC REACTION WHEEL DISTURBANCE SIGNATURE ELIMINATED IN SPECTRUM.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
LAP DISTURBANCE OCCURRING AT CONSTANT FREQUENCIES HAS BEEN ELIMINATED.
DYNAMIC REACTION WHEEL DISTURBANCE SIGNATURE ELIMINATED IN SPECTRUM.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO S/C-COORDS
COORDINATES.DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
INBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

THIS FILE CONTAINS CALIBRATED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE
OUTBOARD MAGNETOMETER ABOARD THE ROSETTA S/C. GROUND CALIBRATION RESULTS HAVE
BEEN APPLIED TO THE RAW DATA. FIELD IS ROTATED TO ECLIPJ2000 COORDINATES.
THE S/C POSITION IS GIVEN IN ECLIPJ2000 COORDINATES AS WELL.
DATA ARE AVERAGED TO 1 S MEANS.

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

HEADER:
FITS header for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation.
IMAGE:
FITS image for Rosetta-Alice calibrated (CODMAC Data Level 3)
histogram observation. Units are photons cm**-2 s**-1 Data are in
units of photons per square centimeter per second
ERROR_IMAGE_HEADER:
FITS extension header
ERROR_IMAGE:
FITS extension containing the statistical uncertainty associated
with each pixel in the primary extension. This is derived by
assuming Gaussian statistics, such that for a given number of
detected counts, N, the corresponding uncertainty is sqrt(N).
Units are photons cm**-2 s**-1 Data are in units of photons per
square centimeter per second
WAVELENGTH_HEADER:
FITS extension header
WAVELENGTH_TABLE:
FITS extension containing the wavelength vector in units of
Angstroms.
PULSE_HEIGHT_HEADER:
FITS extension header
PULSE_HEIGHT_TABLE:
The pulse height distribution (PHD) is a one-dimensional
histogram, that bins each of the detected events (pulses) based on
their 'amplitude'. Detected events are those that are larger than
the discriminator setting, which is an analog (voltage) value. Of
the 16 PHD bins, both the top and bottom 3 bins don't get any
events (this is caused by the digitization of this amplitude
information), so only 10 bins contain non-zero values. The
sampling parameter interval is effectively unknown and somewhat
arbitrary anyway since only the relative shape and stability of
the distribution is of interest.
COUNT_RATE_HEADER:
FITS extension header
COUNT_RATE_SERIES:
These count rate data are a vector that gives the measured count
rate from the observation. Units are counts per time hack interval

This index lists the type, projection,
target body, source mission, and other relevant parameters describing
the maps of small solar system bodies prepared by Phil Stooke of the
University of Western Ontario. The map sheets themselves are provided
in the document directory in the form of jpeg files along with an html
map guide called 00_map_guide.html.